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Black Hole Information Problem and Wave Bursts

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Abstract

By reexamination of the boundary conditions of wave equation on a black hole horizon it is found not harmonic, but real-valued exponentially time-dependent solutions. This means that quantum particles probably do not cross the Schwarzschild horizon, but are absorbed and some are reflected by it, what potentially can solve the famous black hole information paradox. To study this strong gravitational lensing we are introducing an effective negative cosmological constant between the Schwarzschild and photon spheres. It is shown that the reflected particles can obtain their additional energy in this effective AdS space and could explain properties of some unusually strong signals, like LIGO events, gamma ray and fast radio bursts.

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Authors and Affiliations

  1. Javakhishvili Tbilisi State University, 3 Chavchavadze Avenue, Tbilisi, 0179, Georgia

    Merab Gogberashvili & Lasha Pantskhava

  2. Andronikashvili Institute of Physics, 6 Tamarashvili Street, Tbilisi, 0177, Georgia

    Merab Gogberashvili

Authors
  1. Merab Gogberashvili
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  2. Lasha Pantskhava
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Correspondence to Merab Gogberashvili.

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Gogberashvili, M., Pantskhava, L. Black Hole Information Problem and Wave Bursts. Int J Theor Phys 57, 1763–1773 (2018). https://doi.org/10.1007/s10773-018-3702-x

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  • DOI: https://doi.org/10.1007/s10773-018-3702-x

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